Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Crater Floor Outcrop: ESP_067980_2160 ESP_063970_2160 (Interval in Earth days: 312) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.60 | 0.43 | -22. | -12.2 | 54.5 | 59.7 |
| Cross-Cutting Faults Southeast of Melas Chasma: ESP_067732_1650 ESP_073746_1650 (Interval in Earth days: 468) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 290. | -14. | 16.69 | 41.5 | 54.0 |
| Inverted Channel in Cusus Valles: ESP_067833_1960 ESP_067965_1960 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.05 | 49.8 | 5.88 | -3.77 | 43.8 | 44.2 |
| Valleys in Crater Northeast of Argyre Region: ESP_067704_1500 ESP_073784_1500 (Interval in Earth days: 474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.6 | 334. | 7.13 | 20.86 | 44.0 | 53.7 |
| Channels in Orson Welles Crater: ESP_067797_1790 ESP_075433_1790 (Interval in Earth days: 595) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.14 | 314. | 4.35 | -15.7 | 39.8 | 44.2 |
| Floor of Lampland Crater: ESP_068036_1440 ESP_073430_1440 (Interval in Earth days: 421) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.6 | 280. | -4.6 | 13.35 | 52.9 | 59.9 |
| Mounds in Acidalia Planitia: ESP_068074_2280 ESP_068483_2280 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.47 | 312. | -7.6 | 26.38 | 59.5 | 53.0 |
| Collapse Terrain near Orson Welles Crater: ESP_068061_1785 ESP_072677_1785 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.50 | 313. | 1.23 | 21.77 | 41.5 | 55.4 |
| Terrain Sample: ESP_067995_1650 ESP_067520_1650 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 313. | 24.1 | 7.839 | 41.1 | 38.2 |
| Features in Echus Chasma: ESP_068049_1805 ESP_072665_1805 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.707 | 279. | 4.52 | 27.80 | 41.1 | 54.4 |
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